Great Astronomers: Isaac Newton Ball, Robert Stawell
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Service bibliothèque Catalogue historique de la bibliothèque de l’Observatoire de Nice Source : Monographie de l’Observatoire de Nice / Charles Garnier, 1892. Marc Heller © Observatoire de la Côte d’Azur Février 2012 Présentation << On trouve… à l’Ouest … la bibliothèque avec ses six mille deux cents volumes et ses trentes journaux ou recueils périodiques…. >> (Façade principale de la Bibliothèque / Phot. attribuée à Michaud A. – 188? - Marc Heller © Observatoire de la Côte d’Azur) C’est en ces termes qu’Henri Joseph Anastase Perrotin décrivait la bibliothèque de l’Observatoire de Nice en 1899 dans l’introduction du tome 1 des Annales de l’Observatoire de Nice 1. Un catalogue des revues et ouvrages 2 classé par ordre alphabétique d’auteurs et de lieux décrivait le fonds historique de la bibliothèque. 1 Introduction, Annales de l’Observatoire de Nice publiés sous les auspices du Bureau des longitudes par M. Perrotin. Paris,Gauthier-Villars,1899, Tome 1,p. XIV 2 Catalogue de la bibliothèque, Annales de l’Observatoire de Nice publiés sous les auspices du Bureau des longitudes par M. Perrotin. Paris,Gauthier-Villars,1899, Tome 1,p. 1 Le présent document est une version remaniée, complétée et enrichie de ce catalogue. (Bibliothèque, vue de l’intérieur par le photogr. Jean Giletta, 191?. - Marc Heller © Observatoire de la Côte d’Azur) Chaque référence est reproduite à l’identique. Elle est complétée par une notice bibliographique et éventuellement par un lien électronique sur la version numérisée. Les titres et documents non encore identifiés sont signalés en italique. Un index des auteurs et des titres de revues termine le document. -
The Astronomers Tycho Brahe and Johannes Kepler
Ice Core Records – From Volcanoes to Supernovas The Astronomers Tycho Brahe and Johannes Kepler Tycho Brahe (1546-1601, shown at left) was a nobleman from Denmark who made astronomy his life's work because he was so impressed when, as a boy, he saw an eclipse of the Sun take place at exactly the time it was predicted. Tycho's life's work in astronomy consisted of measuring the positions of the stars, planets, Moon, and Sun, every night and day possible, and carefully recording these measurements, year after year. Johannes Kepler (1571-1630, below right) came from a poor German family. He did not have it easy growing Tycho Brahe up. His father was a soldier, who was killed in a war, and his mother (who was once accused of witchcraft) did not treat him well. Kepler was taken out of school when he was a boy so that he could make money for the family by working as a waiter in an inn. As a young man Kepler studied theology and science, and discovered that he liked science better. He became an accomplished mathematician and a persistent and determined calculator. He was driven to find an explanation for order in the universe. He was convinced that the order of the planets and their movement through the sky could be explained through mathematical calculation and careful thinking. Johannes Kepler Tycho wanted to study science so that he could learn how to predict eclipses. He studied mathematics and astronomy in Germany. Then, in 1571, when he was 25, Tycho built his own observatory on an island (the King of Denmark gave him the island and some additional money just for that purpose). -
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere A Constellation of Rare Books from the History of Science Collection The exhibition was made possible by generous support from Mr. & Mrs. James B. Hebenstreit and Mrs. Lathrop M. Gates. CATALOG OF THE EXHIBITION Linda Hall Library Linda Hall Library of Science, Engineering and Technology Cynthia J. Rogers, Curator 5109 Cherry Street Kansas City MO 64110 1 Thinking Outside the Sphere is held in copyright by the Linda Hall Library, 2010, and any reproduction of text or images requires permission. The Linda Hall Library is an independently funded library devoted to science, engineering and technology which is used extensively by The exhibition opened at the Linda Hall Library April 22 and closed companies, academic institutions and individuals throughout the world. September 18, 2010. The Library was established by the wills of Herbert and Linda Hall and opened in 1946. It is located on a 14 acre arboretum in Kansas City, Missouri, the site of the former home of Herbert and Linda Hall. Sources of images on preliminary pages: Page 1, cover left: Peter Apian. Cosmographia, 1550. We invite you to visit the Library or our website at www.lindahlll.org. Page 1, right: Camille Flammarion. L'atmosphère météorologie populaire, 1888. Page 3, Table of contents: Leonhard Euler. Theoria motuum planetarum et cometarum, 1744. 2 Table of Contents Introduction Section1 The Ancient Universe Section2 The Enduring Earth-Centered System Section3 The Sun Takes -
Cu31924002961187.Pdf
iHpil Wd'- !)'..!X;W!iw<il.;! a6 8a. Cornell IDlnivetslt^ OF THE IRew IPorh State CoUeae of agriculture .,%,..x..i:'±e .ii£>\.kho Date Due Library Bureau Cat. No. 1137 Cornell University Library QB 51.B2 Star-land; being talks with young people 3 1924 002 961 187 Cornell University Library The original of tliis bool< is in tine Cornell University Library. There are no known copyright restrictions in the United States on the use of the text. http://www.archive.org/details/cu31 924002961 1 87 STAE-LAND BEING TALKS WITH YOUNG PEOPLE ABOUT THE WONDERS OF THE HEAVENS SIR ROBERT STAWELL BALL, F.R.S. LOWKDEAN PROFESSOR OF ASTEONOMi' IN THE UNIVERSITY OF CAMBRIDGE AUTHOR OF "THE STORY OF THE HEAVENS," ETC. •ffUustrateb NEW AND REVISED EDITION Boston, U.S.A., and London , : ^j GINN & COMPANY, PUBLISHEES die %t\t;mwta. IJreeti 1899 (5155 ,2.z-y-c^ Enteeed at Statiokers' Hall COPYKIGHT, 1899, BY CASSELL & COMPANY, LIMITED ALL EIGHTS KESEKVED (Co THOSE YOUNG FRIENDS WHO HAVE ATTENDED MY CHRISTMAS LECTURES THIS LITTLE BOOK IS DEDICATED PREFACE TO FIRST EDITION. It has long been the custom at the Royal Institu- tion of Great Britain to provide each Christmastide a course of Lectures specially addressed to a juvenile audience. On two occasions, namely, in 1881 and in 1887, the Managers entrusted this honorable duty to me. The second course was in the main a repetition of the first ; and on my notes and recollections of both the present little volume has been founded. I am indebted to my friends Rev. -
Leonhard Euler: His Life, the Man, and His Works∗
SIAM REVIEW c 2008 Walter Gautschi Vol. 50, No. 1, pp. 3–33 Leonhard Euler: His Life, the Man, and His Works∗ Walter Gautschi† Abstract. On the occasion of the 300th anniversary (on April 15, 2007) of Euler’s birth, an attempt is made to bring Euler’s genius to the attention of a broad segment of the educated public. The three stations of his life—Basel, St. Petersburg, andBerlin—are sketchedandthe principal works identified in more or less chronological order. To convey a flavor of his work andits impact on modernscience, a few of Euler’s memorable contributions are selected anddiscussedinmore detail. Remarks on Euler’s personality, intellect, andcraftsmanship roundout the presentation. Key words. LeonhardEuler, sketch of Euler’s life, works, andpersonality AMS subject classification. 01A50 DOI. 10.1137/070702710 Seh ich die Werke der Meister an, So sehe ich, was sie getan; Betracht ich meine Siebensachen, Seh ich, was ich h¨att sollen machen. –Goethe, Weimar 1814/1815 1. Introduction. It is a virtually impossible task to do justice, in a short span of time and space, to the great genius of Leonhard Euler. All we can do, in this lecture, is to bring across some glimpses of Euler’s incredibly voluminous and diverse work, which today fills 74 massive volumes of the Opera omnia (with two more to come). Nine additional volumes of correspondence are planned and have already appeared in part, and about seven volumes of notebooks and diaries still await editing! We begin in section 2 with a brief outline of Euler’s life, going through the three stations of his life: Basel, St. -
Blanchardstown Urban Structure Plan Development Strategy and Implementation
BLANCHARDSTOWN DEVELOPMENT STRATEGY URBAN STRUCTURE PLAN AND IMPLEMENTATION VISION, DEVELOPMENT THEMES AND OPPORTUNITIES PLANNING DEPARTMENT SPRING 2007 BLANCHARDSTOWN URBAN STRUCTURE PLAN DEVELOPMENT STRATEGY AND IMPLEMENTATION VISION, DEVELOPMENT THEMES AND OPPORTUNITIES PLANNING DEPARTMENT • SPRING 2007 David O’Connor, County Manager Gilbert Power, Director of Planning Joan Caffrey, Senior Planner BLANCHARDSTOWN URBAN STRUCTURE PLAN E DEVELOPMENT STRATEGY AND IMPLEMENTATION G A 01 SPRING 2007 P Contents Page INTRODUCTION . 2 SECTION 1: OBJECTIVES OF THE BLANCHARDSTOWN URBAN STRUCTURE PLAN – DEVELOPMENT STRATEGY 3 BACKGROUND PLANNING TO DATE . 3 VISION STATEMENT AND KEY ISSUES . 5 SECTION 2: DEVELOPMENT THEMES 6 INTRODUCTION . 6 THEME: COMMERCE RETAIL AND SERVICES . 6 THEME: SCIENCE & TECHNOLOGY . 8 THEME: TRANSPORT . 9 THEME: LEISURE, RECREATION & AMENITY . 11 THEME: CULTURE . 12 THEME: FAMILY AND COMMUNITY . 13 SECTION 3: DEVELOPMENT OPPORTUNITIES – ESSENTIAL INFRASTRUCTURAL IMPROVEMENTS 14 SECTION 4: DEVELOPMENT OPPORTUNITY AREAS 15 Area 1: Blanchardstown Town Centre . 16 Area 2: Blanchardstown Village . 19 Area 3: New District Centre at Coolmine, Porterstown, Clonsilla . 21 Area 4: Blanchardstown Institute of Technology and Environs . 24 Area 5: Connolly Memorial Hospital and Environs . 25 Area 6: International Sports Campus at Abbotstown. (O.P.W.) . 26 Area 7: Existing and Proposed District & Neighbourhood Centres . 27 Area 8: Tyrrellstown & Environs Future Mixed Use Development . 28 Area 9: Hansfield SDZ Residential and Mixed Use Development . 29 Area 10: North Blanchardstown . 30 Area 11: Dunsink Lands . 31 SECTION 5: RECOMMENDATIONS & CONCLUSIONS 32 BLANCHARDSTOWN URBAN STRUCTURE PLAN E G DEVELOPMENT STRATEGY AND IMPLEMENTATION A 02 P SPRING 2007 Introduction Section 1 details the key issues and need for an Urban Structure Plan – Development Strategy as the planning vision for the future of Blanchardstown. -
A2241: Clusters with Head-Tails at X-Rays L. Norci
A2241: CLUSTERS WITH HEAD-TAILS AT X-RAYS L. NORCI Dunsink Observatory Castleknock, Dublin 15, Ireland L. FERETTI Istituto di Radio Astronomia Via Gobetti 101, 1-40129 Bologna, Italy AND E.J.A. MEURS Dunsink Observatory Castleknock, Dublin 15, Ireland Abstract. A ROSAT Ρ SPC image of the galaxy cluster Abell 2241 has been obtained, showing X-ray emission from the intracluster medium and from individual objects. The brightness distribution of the cluster gas is used to assess the physical conditions at the location of two tailed radio galaxies (in A2241E and A2241W, at different redshifts). Together with radio and X-ray information on the two galaxies themselves the results are of relevance to the question of energy equipartition in radio sources. 1. Background A cluster intergalactic medium plays an important role in determining the morphology and evolution of radio sources. The external gas can interact with a radio source in different ways: confining the source, modifying the source morphology via ram-pressure and possibly feeding the active nucleus. We have obtained ROSAT X-ray data of the region of the cluster Abell 2241, which was previously studied by Bijleveld & Valentijn (1982). A2241 was originally classified as an irregular galaxy cluster, until redshift mea- surements showed it to consist of two separate clusters projected onto each other: A2241W and A2241E, located at redshifts of 0.0635 and 0.1021, respectively. 361 R. Ekers et al. (eds.), Extragalactic Radio Sources, 361-362. © 1996 IAU. Printed in the Netherlands. Downloaded from https://www.cambridge.org/core. IP address: 170.106.33.14, on 29 Sep 2021 at 08:43:38, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. -
Generated on 2012-08-23 18:24 GMT
1SS5 mtt TEGfiNIG. OLD SERIES, NO. II. NEW SERIES, NO. 8. University of Michigan Engineering Society. ALEX. M. HAUBRICH, HEMAN BURR LEONARD, Managing Editor. Business Manager. THOMAS DURAND McCOLL, HOMER WILSON WYCKOFF, CHARLES HENRY SPENCER. THE DETROIT OBSERVATORY OF THE UNIVERSITY OF MICHIGAN. ASAPH HALL, JR., PH.D. This Observatory was built about 1854 through the efforts of Presi- dent Tappan, money for the purpose being raised in Detroit. Mr. Henry N. Walker of Detroit was especially interested in the project and gave funds for the purchase of a meridian circle. The Observatory building is of the usual old-fashioned type, a cen- tral part on the top of which is the dome for the equatorial, and eaBt and west wings, the meridian circle being in the east wing and the library in the west. All the walls are of heavy masonry. About 1853 Dr. Tappan visited Europe and consulted Encke, direc- tor of the Berlin Observatory and Professor of Astronomy in the Uni- versity of Berlin, with regard to the Ann Arbor Observatory. By his advice a meridian circle was ordered of Pistor and Martins and a clock of Tiede. At this time Francis Brunnow was first assistant in the Berlin Obser- vatory. Probably it was through Encke that Brunnow came, in 1854, to- the University of Michigan as the first Professor of Astronomy and. Generated on 2012-08-23 18:24 GMT / http://hdl.handle.net/2027/mdp.39015071371267 Open Access, Google-digitized / http://www.hathitrust.org/access_use#oa-google 10 Thk Technic. Director of the Observatory. 1 think it likely that the 12} inch Fitz equatorial was ordered before his coming; but it was not delivered till after he was on the ground. -
Chapter 1 Chapter 2 Chapter 3
Notes CHAPTER 1 1. Herbert Westren Turnbull, The Great Mathematicians in The World of Mathematics. James R. Newrnan, ed. New York: Sirnon & Schuster, 1956. 2. Will Durant, The Story of Philosophy. New York: Sirnon & Schuster, 1961, p. 41. 3. lbid., p. 44. 4. G. E. L. Owen, "Aristotle," Dictionary of Scientific Biography. New York: Char1es Scribner's Sons, Vol. 1, 1970, p. 250. 5. Durant, op. cit., p. 44. 6. Owen, op. cit., p. 251. 7. Durant, op. cit., p. 53. CHAPTER 2 1. Williarn H. Stahl, '' Aristarchus of Samos,'' Dictionary of Scientific Biography. New York: Charles Scribner's Sons, Vol. 1, 1970, p. 246. 2. Jbid., p. 247. 3. G. J. Toorner, "Ptolerny," Dictionary of Scientific Biography. New York: Charles Scribner's Sons, Vol. 11, 1975, p. 187. CHAPTER 3 1. Stephen F. Mason, A History of the Sciences. New York: Abelard-Schurnan Ltd., 1962, p. 127. 2. Edward Rosen, "Nicolaus Copernicus," Dictionary of Scientific Biography. New York: Charles Scribner's Sons, Vol. 3, 1971, pp. 401-402. 3. Mason, op. cit., p. 128. 4. Rosen, op. cit., p. 403. 391 392 NOTES 5. David Pingree, "Tycho Brahe," Dictionary of Scientific Biography. New York: Charles Scribner's Sons, Vol. 2, 1970, p. 401. 6. lbid.. p. 402. 7. Jbid., pp. 402-403. 8. lbid., p. 413. 9. Owen Gingerich, "Johannes Kepler," Dictionary of Scientific Biography. New York: Charles Scribner's Sons, Vol. 7, 1970, p. 289. 10. lbid.• p. 290. 11. Mason, op. cit., p. 135. 12. Jbid .. p. 136. 13. Gingerich, op. cit., p. 305. CHAPTER 4 1. -
PDF < Theory of Screws: a Study in the Dynamics of a Rigid Body (1876
Theory of Screws: A Study in the Dynamics of a Rigid Body... ~ PDF ^ ILWU0YQOFY Theory of Screws: A Study in the Dynamics of a Rigid Body (1876) by Robert Stawe By Robert Stawell Ball Createspace Independent Publishing Platform, United States, 2016. Paperback. Book Condition: New. 229 x 152 mm. Language: English . Brand New Book ***** Print on Demand *****.Sir Robert Stawell Ball FRS (1 July 1840 - 25 November 1913) was an Irish astronomerwho founded the screw theory He was the son of naturalist Robert Ball[2] and Amelia Gresley Hellicar. He was born in Dublin. Ball worked for Lord Rosse from 1865 to 1867. In 1867 he became Professor of Applied Mathematics at the Royal College of Science in Dublin. There he lectured on mechanics and published an elementary account of the science. In 1874 Ball was appointed Royal Astronomer of Ireland and Andrews Professor of Astronomy in the University of Dublin at Dunsink Observatory. Ball contributed to the science of kinematics by delineating the screw displacement: When Ball and the screw theorists speak of screws they no longer mean actual cylindrical objects with helical threads cut into them but the possible motion of any body whatsoever, including that of the screw independently of the nut. READ ONLINE [ 5.33 MB ] Reviews I actually began looking over this pdf. This can be for all those who statte there was not a worthy of reading through. I am easily can get a enjoyment of reading through a written publication. -- Rafael Feeney Jr. Great electronic book and useful one. Better then never, though i am quite late in start reading this one. -
Deriving Kepler's Laws of Planetary Motion
DERIVING KEPLER’S LAWS OF PLANETARY MOTION By: Emily Davis WHO IS JOHANNES KEPLER? German mathematician, physicist, and astronomer Worked under Tycho Brahe Observation alone Founder of celestial mechanics WHAT ABOUT ISAAC NEWTON? “If I have seen further it is by standing on the shoulders of Giants.” Laws of Motion Universal Gravitation Explained Kepler’s laws The laws could be explained mathematically if his laws of motion and universal gravitation were true. Developed calculus KEPLER’S LAWS OF PLANETARY MOTION 1. Planets move around the Sun in ellipses, with the Sun at one focus. 2. The line connecting the Sun to a planet sweeps equal areas in equal times. 3. The square of the orbital period of a planet is proportional to the cube of the semimajor axis of the ellipse. INITIAL VALUES AND EQUATIONS Unit vectors of polar coordinates (1) INITIAL VALUES AND EQUATIONS From (1), (2) Differentiate with respect to time t (3) INITIAL VALUES AND EQUATIONS CONTINUED… Vectors follow the right-hand rule (8) INITIAL VALUES AND EQUATIONS CONTINUED… Force between the sun and a planet (9) F-force G-universal gravitational constant M-mass of sun Newton’s 2nd law of motion: F=ma m-mass of planet r-radius from sun to planet (10) INITIAL VALUES AND EQUATIONS CONTINUED… Planets accelerate toward the sun, and a is a scalar multiple of r. (11) INITIAL VALUES AND EQUATIONS CONTINUED… Derivative of (12) (11) and (12) together (13) INITIAL VALUES AND EQUATIONS CONTINUED… Integrates to a constant (14) INITIAL VALUES AND EQUATIONS CONTINUED… When t=0, 1. -
Gravity, Orbital Motion, and Relativity
Gravity, Orbital Motion,& Relativity Early Astronomy Early Times • As far as we know, humans have always been interested in the motions of objects in the sky. • Not only did early humans navigate by means of the sky, but the motions of objects in the sky predicted the changing of the seasons, etc. • There were many early attempts both to describe and explain the motions of stars and planets in the sky. • All were unsatisfactory, for one reason or another. The Earth-Centered Universe • A geocentric (Earth-centered) solar system is often credited to Ptolemy, an Alexandrian Greek, although the idea is very old. • Ptolemy’s solar system could be made to fit the observational data pretty well, but only by becoming very complicated. Copernicus’ Solar System • The Polish cleric Copernicus proposed a heliocentric (Sun centered) solar system in the 1500’s. Objections to Copernicus How could Earth be moving at enormous speeds when we don’t feel it? . (Copernicus didn’t know about inertia.) Why can’t we detect Earth’s motion against the background stars (stellar parallax)? Copernicus’ model did not fit the observational data very well. Galileo • Galileo Galilei - February15,1564 – January 8, 1642 • Galileo became convinced that Copernicus was correct by observations of the Sun, Venus, and the moons of Jupiter using the newly-invented telescope. • Perhaps Galileo was motivated to understand inertia by his desire to understand and defend Copernicus’ ideas. Orbital Motion Tycho and Kepler • In the late 1500’s, a Danish nobleman named Tycho Brahe set out to make the most accurate measurements of planetary motions to date, in order to validate his own ideas of planetary motion.